What exactly is Weinberg's power counting theorem? 
The massive gravity propagator goes like $\sim \frac{p^2}{m^4}$ at
  high energies and in this case we cannot apply Weinberg's standard
  power counting arguments.

I have read something like that in an article but didn't understand what is Weinberg's power counting arguments and how to use them. The original article of Weinberg, with the title "High-Energy Behavior in Quantum Field Theory", is too complicated for me. Can anybody explain this method in a more simpler way?
 A: Let's look at the analog of the massive photon. The propagator for this is
$$
\frac{ g^{\mu\nu} - \frac{p^\mu p^\nu}{m^2}  }{ p^2 + m^2 } 
$$
At large energies, this scales like $\frac{p^\mu p^\nu }{m^2 p^2} \sim \frac{1}{m^2}$. 
In the same way, the massive graviton propagator takes the general form
$$
\frac{g^{\mu\alpha} g^{\nu\beta} + g^{\mu\beta} g^{\nu\alpha} - \# g^{\mu\nu} g^{\alpha\beta} + \# \frac{ p^\mu p^\alpha }{ m^2 } g^{\nu\beta} + \# \frac{ p^\nu p^\beta }{ m^2 } g^{\mu\alpha}  + \# \frac{ p^\mu p^\nu }{ m^2 } g^{\alpha\beta}  + \# \frac{ p^\alpha p^\beta }{ m^2 } g^{\mu\nu}  + \# \frac{p^\mu p^\nu p^\alpha p^\beta }{ m^4 } }{p^2 + m^2 }   
$$
where $\#$ are numbers whose values I cannot recall off the top of my head. They are fixed by requirements that when contracted with $p_\mu$ or $p_\nu$ or $p_\alpha$ or $p_\beta$ or $g_{\alpha\beta}$ or $g_{\mu\nu}$ it vanishes. 
At high energies, this propagator scales like
$$
\frac{p^\mu p^\nu p^\alpha p^\beta }{ p^2 m ^4 } \sim \frac{p^2 }{ m^4 } ~. 
$$
